Image Details
Caption: Figure 10.
ASXDF1100.053.1 SED at observed optical/near-/mid-IR wavelengths. Top: Best-fit SEDs, ignoring emission lines, for z = 5.5, 6.5 and 7.5, as obtained with Le Phare. Black points correspond to the observed flux densities, while arrows indicate 2σ upper limits. Bottom: Best-fit SEDs, this time including emission lines.
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